Pith. sign in

REVIEW 4 cited by

Parameter estimation for Galactic binaries by LISA

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0204487 v1 pith:YEJTDGAW submitted 2002-04-29 astro-ph gr-qc

Ryuichi Takahashi , Naoki Seto This is my paper · ORCID
classification astro-phgr-qc
keywords binariesgravitationallisalsimparameterswaveaccuratelyanalysis
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We calculate how accurately parameters of the short-period binaries $(10^{-4} {Hz} \lsim f\lsim 10^{-2} {Hz})$ will be determined from the gravitational waves by LISA. In our analysis the chirp signal ${\dot f}$ is newly included as a fitting parameters and dependence on observational period or wave frequency is studied in detail. Implications for gravitational wave astronomy are also discussed quantitatively.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Probing the Orientation Distribution of Nearby Double White Dwarfs through Gravitational Waves with LISA

    astro-ph.GA 2026-07 conditional novelty 6.0 of 10

    A spherical-harmonic method extracts low-multipole orientation coefficients of ~500 nearby double white dwarfs from LISA data with ~0.02 shot-noise uncertainty.

  2. A Multimessenger Strategy for Downselecting the Orientations of Galactic Close White Dwarf Binaries

    gr-qc 2025-07 accept novelty 6.0 of 10

    Using EM-determined orbital phases, the fourfold degeneracy in the transverse projection of a close white dwarf binary's angular momentum from LISA data can be reduced to a twofold degeneracy.

  3. Eccentric Stellar-mass Binary Black Holes: Population, Detectability, and Waveform Analysis in the LISA and LIGO Era

    astro-ph.HE 2026-05 unverdicted novelty 5.0 of 10

    Simulations of dynamically formed eccentric stellar-mass BBHs predict dozens of LISA-detectable sources in the Milky Way, hundreds of low-SNR extragalactic mHz sources, a merger rate of ~9 Gpc^{-3} yr^{-1}, and potent...

  4. Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization

    astro-ph.IM 2025-10 unverdicted novelty 5.0 of 10

    Simulations of continuous-wave searches show that PTA data first constrain GW frequency and strain amplitude together, then sky location, with chirp mass and inclination following later for evolving sources, with prec...

Pith tools